Published November 22, 2022 | Version v1
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Internal proper motion dispersion profiles for 37 Milky Way globular clusters extracted from Gaia EDR3

  • 1. Saint Mary's University
  • 2. University of Queensland
  • 3. ICREA, University of Barcelona

Description

Internal proper motion dispersion profiles, in the radial and tangential components, extracted from Gaia EDR3 data for 37 Milky Way globular clusters.

Created for, and used for model fitting in, the submitted manuscript: "Multimass modelling of Milky Way globular clusters - I. Implications on their stellar initial mass function above 1 M$_{\odot}$". Details on the creation of this dataset are available within this article.

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